Optical system



BEQ QQZ SR 229m KR 29199:;(314- April 23, 1940. H. G. OTT (43 OPTICAL SYSTEM Filed Jul 22, 1957 2 Sheets-Sheet 1 ATTORNEYS A ril 23, 1940.

H. G. OTT OPTICAL-SYSTEM Filed m 22, 1937 2 Sheets-Sheet 2 INVENTOR (0% ATTORNEYS semen stares 2,198,014 OPTICAL SYSTEM Harry G. Ott, Kenmore, N. Y. Application July 22, 1937, Serial No. i,991

This invention relates to optical systems and more particularly to an image formingdevice for an optical system such as may be employed, by way of example, in headlights of motor ve- 6 hicles, in optical projection appar atus and as an objective of a microscope.

One object of the invention is to provide an improved optical system for forming an image of a source of light, having a large angular apso erture heretofore unattainable with freedom a given source may be obtained on a given area,

with which glare to approaching drivers may be eliminated or reduced to such an extent as to 1 he non-objectionable, which will not materially increase thespace occupied by present day headlights, and which will be relatively simple and inexpensive.

Other objects and advantages will be apparent from the following description of several em- 39 hodiment's of the invention, and the novel features will be particularly pointed out hereinafter in connection with the appended claims.

in the accompanying drawings: Fig. 1 is an optical diagram illustrating optical principles and explaining some of the basic equations referred to in the specification;

Fig. 245 a sectional elevation through a motor vehicle headlight constructed in accordance with this invention, and illustrating one application of the broad features of the invention; Fig. 3 is an optical diagram illustrating the applicationo'i the invention to an optical pro-U jection condensing system, such as for motion picture machines or stereoptican projection deg ices;

'ig. 4 is an optical diagram illustrating the application of the invention to image magnifying devices, such as a microscope, where the im' proved system is used as the objective of the magnifying device; and

Figs. 5 and 6 are diagrams illustrating other applications of the same improved optical system. In optical systems for the creation of an image of a source of. light, if a large angle of illumt- 5 nation at the source is used, considerable dim- -approaching car.

9 Claims. (CI. 88-24) culty has been encountered in bringing all of the rays of light from the source accurately to a focus to form an image of the source, with the result that the image is either blurred or if the source of light is afilament the image includes 5 an area of concentrated light and an encircling area of lesser intensity which is caused by spherical aberration and/or coma. Throughout this specification and claims, a source of light is considered to include a primary or initial source of light, such as a filament of an electrlc'lamp or the center of an arc in an arc lamp, or an object illuminated from an exterior source, the light rays reflected from which object are brought to a focus so as to form an image of the illuminated object. In a headlight or projection device, the source oi light will, of course, be the filament or primary source of light, whereas in'a magnifying device, such as a microscope. the source of light will be the illuminated object to be magnified, and the expression source of light" in the claims is to be interpreted in accordance with this exiflanation.

The size of an image formed by an optical system is dependent upon the focal length of 25 the system. The focal length of any system will vary over its aperture if the optical aberration, known as coma, is not corrected. To illustrate,

a simple lens system may be corrected for spher ical aberration, and thereiore form an image in 30 the same place by both the central zone and the annular peripheral zone of the lens, but if coma or sine condition is not corrected, these two zones will form images of difierent sizes.

In lens systems, the difference in focal length 35 for difierent zones across the aperture is a small percentage of the axial focal length. in the parabolic reflector, however, the variation in focal length for difierent zones is great, running up to two or three hundred percent. This means i that in a headlight using a parabolic reflector, the outer zones of the reflector form images of the--=filament on the road that are one-half to one-third the size of the image formed by the axial zone. Since the greatest concentration or light is at the center of this series of overlapping images, this portion must he directed on the road at a considerable distance from the car. 'When this is done, the larger images are large enough to throw-light into the eyes of the driver of an 50 it is this sine condition or coma error of the parabolic reflector that mairm the problem of glare control so acute, since the parabolic reflector, corrected for spherical aberration, which means that all of its zones form an image of the filament at infinity, is almost universally used. The lenses used in conjunction with the parabolic reflector are attempts to corroot the bad effect introduced by the coma error, although in the usual headlight engineering parlance, this is not so stated. That these lenses are only a partial solution to the problem seems evident on casual observation.

The glare problem can be solved, if an optical system can be designed that will put enough light on the road, in a properly restricted area. Such an optical system must be corrected for both spherical aberration and coma or sine condition. The size of the area illuminated can be controlled by the size of the filament and the focal length of the optical system, since the image of the filament is formed far enough away from the car to be considered at infinity with reference to the optical system. Because of the fact that the 138.11 (la-Ft!!!) a tan 01 /1-l-tan a /1+tan (25"tB-D. a; tan a +1 If a is the distance from A to A, and A is chosen as the center of coordinates, then r (Who- 4) (aa) (a-yl) filament is small in comparison to the focal length of the optical system, a correction for. both spherical abberration and coma'insures' a good image of the filament on the road. It follows that all of the light will pass through this image, and none will wander outside its limits. Therefore, if the image is of such a size and so directed as to illuminate the road, but at a height below the eyes of the approaching driver, no light will enter his eyes and cause glare.

In the practice of my invention, I'use what may be termed a double reflecting system, in which substantially all the utilized light from the source is subjected to at least two reflectionsin forming the image. I will, therefore first discuss those principles of such double reflection which have to do with this invention.

These double reflecting systems utilize two reflecting surfaces, P and Q (Fig. 1) small sections only of which are shown in the drawing. By means of these two surfaces, light is directed from the point or source A to the image or point The first condition which requires reflection from A to A. can be stated mathematically from the well known law of reflection in the two equations:

with due regard to the signs of the angles.

The tangents of a and 01 are the slopes of the two surfaces at the points in question, and are therefore the dy/dr .of these two curves.

Expanding Equations 1 and 2 in terms of the tangents of the angles, the following equations are obtained.

an m /1+tan a, /1-1-tan ar -tan a tan 042+ In this manner two equations in the rectanglar coordinates of the two unknown curves are obtained, each equation containing the coordinates of both curves. To obtain a solution to the problem it is necessary to obtain two equations, the one containing only the coordinates of theone curve and the other only the coordinates of the other curve. At present there are only two equations with five variables, since a will vary for each ray, and three of these five variables, must be eliminated. Therefore, two more equations, orv conditions, are required to reach a discrete solution. These two conditions can be chosen at will. If ease of manufacture'is of first importance, then probably-the best choice is to designate each surface as a sphere, or circle in the plane of the diagram, since the spherical surface is much the easiest of all surfaces to manufacture.

If, however,'perfection of image formation a. the-point A is a major requirement, then the condition of correction of one or two of the well known optical' aberrations can be imposed. If only one-aberration is corrected, either one of the reflectors can-be made a sphere, and the other will be of a shape indicated by the equation derived after the desired condition, is stated mathematically andv proper and necessary elizni- 55 where b and c are the distances from A of the centers of the two circles, and r has its usual meaning. This may appear to be a statement of the solution to the problem at the start, since expressions for the shapes of the two reflectingsurfaces are the requirement of this work. It is, however, possible to eliminate three of the four 11's and y's between Equations 5, 6, 7 and 8 and thereby obtain an expression involving a, and theother a: or 1 which would give an indication of the spherical aberration'of the system. With certain values of the constants, b, 0, T2, T4 the variation 'of a would be small enough to make a practical system. i This is shown by the fact that one type of dark field illuminator now on the market consists of such a reflecting system composed of two spherical surfaces. In general, however, such a system is usable only for narrow limits of the values of the constants and also for a relatively limited range of values of a1. wherever its application requires a reasonably good optical correction.

If the optical aberration commonly known as spherical aberration is corrected, not only must a. be a constant, but also the total length of path from A to A must be equal for all possible paths,

1/(= 4 )+y4 =K1 where K1 is a constant, and this becomes one of the two additional conditions needed'ior a discrete solution. I The other condition can be chosen at will. Making either one of the two surfaces a sphere would probably be desirable. A system meeting conditions 5, 6 and 9 would produce a good image, of the point A at A. It would not, however, necessarily produce a good image at A of an object having finite size even though the object should be very small. In order to produce a good image of a finite but small object the coma or conditionknown as the sine condition must be met. Stated mathematically, the sine y 2\ 4 fi -i U4 w 412w: or-if a is infinite, the sine condition becomes In some cases it might be desirable to have Ki, & or K3, or any combination, vary rather than remain constant. This variation can be expressed as any arbitrary function 0! any of the variables in the problem. If an is chosen as the variable, then the most general form of expressionis a where 'i(m2), fafirz) and fa(:rz) are any arbitrary functions .of 2:2 that may be chosen to meet conditions imposed onthe problem, and K0. Mo and F0 are initial values of these quantities, these values also being arbitrarily designated to meet desired conditions.

Equations 5, 6, 14 and 15 give a complete solution to the problem of designing two reflecting surfaces having any desired correction for both spherical aberration and sine condition. It A is in finite space, expressions for $4 and 3 4 can be obtained from 14 and 15 and these put into 5. This will result in a differential equation for the larger curve. This equation must be integrated and solved, point by point to plot the curve. A corresponding procedure will give the other curve. This is an extremely complicated procedure. It is quicker and easier to use the following method to get'the coordinates of these curves.

When zrz=0 m1=90 sin ai -1.0

and Equation 15 becomes Since the process of eliminating the variables mentioned above results in a differential equation, another constant will be introduced when this equation is integrated. This constant can be taken as the value oi 14 when 322:0. Let this be designated by 1:. Then This designates three of the four coordinates. The value of ya can be computed from 14, or, since the numerical value of f1($2)Ko may not be of any real importance at this point, n can be given an arbitrary value and the starting value of f|(:c2)Ku can be determined .by 14. This gives a point on each curve to meet the condition of correction for sine condition and spherical aberration. It remains to make these two points meet the necessary condition of reflection, as expressed in 5 and 6, but also expressed in l and 2 in simpler terms. as has been designated as Equations 19 and 21 require these points on each curve to meet the conditions of reflection'as stated in Equations 1 and 2, and they'are therefore points on the pair of curves, the pair meeting the conditions stated in Equations 1, 2, 14 and 15. These are points on the curves that are the loci of the two equations that could be derived from the four Equations 5, 6, l4 and 15 as Equations 20 and 22 afford the means of proceeding to the next point. Since the start of the method was the designation of the initial value of 1:2, an arbitrary value of CD12 in Equation 20 is used, and since the value of tan a2 is known, the value of (1112 can be computed. This is used as though it correctly designated the new 312. This is not strictly correct, since this 112 is on the tangent to the curve at the starting point, and therefore lies off the true curve by the amount that this tangent recedes from the curve at the new value of $2. This error is disregarded at first and corrected later in a manner to be described.

From the work already done the first ten as can be computed by Since the'new a: and 11/2 are now known, the new sin 411 can be computed by tan a 1 /2 .Sln (X1:

was:

and the new sin as by sin a IMMI.

From this the value of tan as can be obtained,

and subtracted from the previous value of tan (:5 to get d (tan as) Since (Q74 0) (1038.11 (15) tan a tan us These last two equations of 6334 and dyi give the means of getting the new point on the small curve, at; and 1/4.

This pair of newpoints meets three of the four conditions stated, since the new a: and 124 are computed as before to meet the conditions of reflection, and the sine condition correction is obtained by virtue of the method used. There is, however, nothing in this method to insure that these points will satisfy Equation 14, which is a statement that the spherical aberration is to be corrected. The next step is to put these new values of the coordinates in Equation 14 and compute the new value of f1(I1!2)Ko. Because of the error mentioned above, this new value will be slightly in error. A small arbitrary correction to dyz must be made, and the process repeated, until the value of f1(:I.2)Ko is close enough to the required value for all practical purposes.

After this has been done a few times for several points the proper amount of correction to give to dyz can be estimated with ease.

When the proper correction to dyz is found, this new pair of points-lie on the pair of curves that satisfy the four conditions stated, and the remarks at the top of page apply here also. In this way the whole pair of curves can be derived, with as much accuracy as though a single equation for each curve were developed and I solved, and with much less work.

obvious simplifications of the equations and procedure. f1(:cz) and fz(:c2) are given the constant value of one. The value of :2:, which positions the two curves with respect to each other is given a value of mm., and F0 is made 20 mm. The value of y: when u1=90 is 40 mm.

It should be noted that when this process is carried to its ultimate conclusion of a perfect correction, an optical system is obtained that is perfectly corrected for spherical aberration and sine condition, and since only reflections are involved it is also perfectly corrected for color, and these perfect corrections cover an extremely large angular aperture. This is a definite improvement over the usual lens system type of image forming device, since all lens systems suffer from small residual aberrations that cannot be-eliminated, and when the angular aperture is large these residual aberrations cause a noticeable deterioration of the quality of the image.

This system is a definite improvement over the usual types of reflecting systems used in some sin a S111 (1 K it is seen that when on changes sign, 015 must also change sign if K is to remain constant. This, in turn, means that A must lie to the left of the small curve instead of as shown in the figure. To accomplish this, the slope of the small curve must change abruptly. In other words there is a point of discontinuity at the point on the small curve corresponding to the point on the large curve where oz1=90. If on is changed in one direction from this value, one set of curves is obtained, and quite a different set if a1 is changed in the other direction. There are, therefore, at least two classes of combinations of these curves. The first is illustrated by Figs. 2, 3-and 4 and the second by Fig. 5.

The differentiation between these two classes lies in the fact that in Figs. 2, 3 and 4 the object and image are on opposite sides of the small curve and in Fig. 5 they lie on the same side. Perhaps a. more significant differentiation lies in the fact the first quadrant and in Fig. 5 all values of'i' lie in the second quadrant. Since object and image are interchangeable, the point A must be defined as the point furnishing light to the large mirror, and A the point furnishing light to or receiving it from the small mirror.

.If the point A is moved to the right, beyond the small reflector, in Fig. 5, the combination as shown in Fig. 6 is obtained.

If the point A is moved to the right to infinity, this is a combination useful for telescopes. It should be noted here that there is another, equally valid, way of designating-the difference between Figs. 2 to 4 and Fig. 6. If the point A in Figs. 2 and 3 is moved out to the left, the useful part of the larger reflector at its right-hand end motor vehicles.

cal

. gram that is reversed right and left from Fig. 6.

When the above alterations of Figs. 2 and 3 are made, and point A moved to the left to infinity,

a combination suitable for telescopes is again reached. 7 All three of these classes of combinations can be altered to make the light rays from the larger reflector cross the axis before striking the small reflector. Such procedure serves to invert the image, and such combinations are useful wherever this is desired. In this case the small reflector becomes concave instead of convex. If this is done for the arrangement of Figs. 2 to 4, only 180 about the axis can be used or otherwise one half of the small reflector would shield the light from the other half.

Referring now to Fig. 2, I have illustrated one application of the invention to a headlight for In' that embodiment of the invention, the improved headlight includes a casing it of any suitable construction and of any desired shape. The source of light is a filament ii of an electric light bulb i2 which is supported in any suitable or usual manner by a socket 13' that in turn is supported in any suitable manner, such as from the removable rear wall I :i of the housing. The front wall of the housing is provided with a suitable window or aperture l5 through which light from the source H is projected. A semi-sphericaL-concave mirror It is disposed about the socket i3 at the rear of the housing, and the center of curvature of the inner face of the mirror is substantially at the center of the filament H. Therefore, any light rays from the filament I l which, upon leaving the fllament travel rearwardly and impinge upon the mirror It, will be reflected by the spherical mirror is back along the same radius to that mirror, and through the filament and thence forwardly in the housing l0.

Within the housing ii! is a relatively large, concave reflector or mirror I? which may be tubular and have a surface of revolution, although this invention is not limited to a surface of revolution, for in some cases a departure from such a surface is desirable, the axis of revolution of which is substantially coincident with the line between the center of the filament II and the center of the aperture or window I5. This concave reflector I! preferably extends at one end approximately to a plane through the filament ii and normal to the axis of revolution of the reflecting surface of reflector 11. The particular curvature of the reflecting surface of this cancave tubular reflector is selected or determined by the method hereinbefore exp1ained.'

Within the housing l0 but further along the axis of reflector I! is a second and smaller, but convex reflector i8 which is disposed across said axis adjacent to the aperture i5, and this convex reflector it also has a surface of revolution, with its axis coincident with the axis of generationof'' the reflector l1, as its reflecting surface, and progressing generally in the same direction as the axis of reflector l'i. Thus the convex reflector I 8 is within and has its reflecting surface facingthe tubular concave reflector l'l, adjacent the aperture i5. I

This reflector l8 may be supported in any suitable manner, such as by having at its smaller or 'forward end, a small stud IQ which extends araaom ture l5 and through a small spider frame or transparent plate 2|! carriedby the front end of the housing l0 and spanning the aperture or window l5. This frame 20 supports the reflector I8 and if a spider, it should be as small as possible soas to obstruct the passage of only a minimum of light,'or, if desired, it can be so shaped and positioned as to reflect, refract or direct some light out of the path directed by the optical system, but if it is a plate of glass, it serves to close the front end of the housing, that is, the aperture or window l5 therein. That end of the convex reflector l8 which is nearest the source of light I I may be made of any desired curvature, but it is preferably coated; with a light absorptive coating so that any light rays striking the same will be largely absorbed instead. of

reflected.

Typical light rays L1, L2, L3, L4, L5, are illustrated, by way of example, as leaving the fllament H, and the paths of such rays are indicated in,

strikes the concave reflector I! intermediate of its ends and is reflected thereby inwardly and forwardly against the convex reflector l8 and thence forwardly through the aperture or window !5 at the front of the housing. The ray L2 strikes the concave reflector IT at the rearward end thereof, and is reflected forwardly thereby against the rear or innermost end of the reflector l8, and thence'forwardly through the aperture or window it. The light ray In leaving the fllament H and passing forwardly at a small angle to the axis of the reflector -il just clears the rear or inner end of the reflector l8 and strikes the forward end of the reflector ii and is there reflected backwardly against the forward end of the reflector i8, and thence forwardly through the aperture or window it.

The light ray L4 is an example of that small bundle of the light rays which leave the fllament l i and directly impinge upon the inner end 2i of the reflector l8, and such rays are either absorbed orreflected back to the fllament. Preferably this end wall 2! is made partially spherical, with the center of curvature at the fllament, so that if any of the rays of light impinging on this surface 2i are not absorbed they will be reflected back to the fllament instead of being reflected to the reflector H where they might be reflected in a manner that would cause them to leave the window i5 and cause glare. The light rays, of which L5 is an example, which leave the filament H and pass rearwardly to impinge upon the semi-spherical reflector it will, by reason of the fact thatthe center of curvature of that reflector is at the fllament, be reflected back to the fllament and thence will travel in a manner forwardly to impinge upon the reflector l I in the same manner as though those light rays had originally travelled forwardly in the same direction from fllament H. Thus, the ray L5 after reflection will travel forwardly along with the ray L1, for example.

From these examples it will be observed that all the rays of light from the fllament it which are allowed to leave the window or aperture I5 of the housing will be subjected to at least two major reflections, one by the concave reflector ii to the convex reflector I8, and then by the latter forwardly through the aperture or window i5 of the housing. If the curvature githe reflectqliLan Lh 8-,is corrected i or spherical V mam and also for coma orisine condition animate" a naxin um concentration of light so that maximum but controlled illumination will be obtained by this device.

It will be observed that the forward end of reflector ll subtends a bundle of light rays from the filament which is substantially the same bundle which is subtended by the inner end surface 2l of reflector [8, so that substantially no direct and unreflected light rays from the filament can escape through the window l5 and cause glare. It'will also be noted that the reflector l1 hasa relatively large reflecting surface and subtends a relatively large angle at the filament, and that the reflector l8 has a relatively small reflecting surface and subtends a relatively small angle at the filament.

It will also be observed that the reflector with the convex face subtends a relatively small angle at the source or the filament, and has a relatively small angular aperture at the image of the source; also that the reflector with the concave face subtends a relatively large angle at said source or filament. The angular aperture is the angle formed at the axial point of the object or image between the axis and the ray having the greatest inclination to the axis, that can enter or leave the system, providing none of the rays between the axis and this extreme ray are obstructed by the system. If such an obstruction occurs, then the angular aperture is the angle of the hollow cone of rays permitted to enter or leave the system.

In Fig. 3 the application of this type of device to an optical projection system is illustrated. In this embodiment of the invention the source of light and the reflectors may be provided, the same as in Fig. 2, except that the reflected rays leaving the convex reflector l8 will be more convergent and brought to a focus approximately at the projection lenses 22. The converging light rays pass through any lantern slide or film at the aperture or frame D and then through the usual projection lens device 22 so as to project an image of the slide or film upon a screen, as usual in optical projection apparatus of this type.

In Fig. 4 the application of this invention to a magnifying device, such as a microscope, is illustrated. Light from any suitable source is concentrated upon an object mounted on a microscope slide 24, in any suitable manner such as by means of the usual microscope condensing system 25, and the object on the slide 24 which is thus illuminated corresponds to the source of light provided by the filament H in the optical system of Figs. 2 and 3. It is the light rays re-' fiected by the object so illuminated that are doubly refiectedmby the reflectors I! and 18in ,microscopes and the like.

Other applications of the invention will be apparent to those skilled in the art from the foregoing examples, and it will be observed that unusually complete control of the light rays is obtained and maximum concentration of light at the focus is obtained in all of the various applications.

In Figs. 5 and 6, difierent arrangements of the reflectors l1 and I8 are illustrated diagrammatically, the arrangement on only one side of the optical axis of the system being shown, so that it will be understood that in practice, the reflectors may extend on both sides of the axis in the same manner.

It will be understood that various changes in the details which have been herein described and illustrated in order to explain the nature of the invention may be made by those skilled in the art within the principle and scope of the invention, as expressed in the appended claims.

I claim:

1. An image forming device for an optical system, such as for light projecting devices and microscope objectives, comprising an outer concave mirror and a smaller convex mirror, a source of light disposed at a finite distance from said concavemirror, said concave mirror subtending a relatively large angle at said source and said convex mirror subtending a relatively small angle at said source and having a relatively small angular aperture at the image of said source, the mirrors forming an optical system upon an optical axis and being of such a shape that the curves formed by the intersection of the surfaces and a plane through the axis consist of corresponding pairs of points, each pair satisfying the conditions expressed by the equations;

and

M: M (a constan 114 1/:E+ Z1:

fi- JZZ-iy,: F (a constant) when a is infinite, and the slopes of the curves at these points being such that curve,

on is the angle between said optical axis and.,.

a ray of light from said source and directly incident on said concave mirror,

. a2 is the angle betweenthe tangent to the concave mirror at the point of incidence thereon of said ray and a parallel to said optical axis,

as is the angle between the ray of light reflected from said concave mirror and said optical axis,

a4 is the angle between the tangent to the convex mirror at the point of incidence thereon 0f the reflected ray of light from said concave mirror and said optical axis, and

a is the distance from said source to said image.

2. An image forming device for an optical system comprising an outer concave mirror and a smaller convex mirror, a source of light disposed 7 at a finite distance from said concave mirror, said concave mirror subtending a relatively'large angle at said source and said conve'x mirror subtending a relatively small angle at said source and having a relatively small angular aperture flit/madam at tlese points being such that (a;+as)

in wlich equations:

2:2 and y: are the coordinates curve, $4 and 114 are the coordinates of the convex curve, Y s1 is the angle between said optical axis and of the concave 51' ray of light. from said sourceand directly incident on said concave mirror,

(:2 is the-angle between the tangent to the coni 35 cave mirror at the point of incidence thereon or said my and a parallel to said optical axis,

as is the angle between the ray 01 light reflected from said concave mirror and said optical axis,

a4 is the angle between the tangent to the coni vex mirror at the point of incidence thereon of he eflected ray 02 light from said concave mirror aid optical axis, i a is the distance from said source to said image, his-l) awn and f3($2) are any arbitrary funcd5 imposed on the problem, and

' Mo and 2% are initial values of these quantities arbitrarily designated to meet desired conditions.

3. An image forming device for an optical systom comprising a pair of spaced reflecting surfaces, 0, source of light disposed at a finite distance from of said reflecting surfaces, said one surface suctending a relatively large angular aperture at said source, and the other of said surfaces subheading a. relatively small angle at said source and having a relatively small angular aperture at the image of said source, the two the approximate loci oi the difierentiel equations- :5 curve, and

"having said source in said axis at oneiocus in spherical aberration, and coma 20' the sine condition, in the im "he; a is infinite, and the slopes or the curves age vfirst from one reflector and then from the otherreflector to said image, said source being finite of $21 that may be chosen to meet conditions suriaces being in a plane section through the axis,

l 7 duo, d212, (111 and dm are increments of change of an, 11:, x4 and 114' respectively:

4. An improved, image forming optical device comprising a source of light, a double reflecting,

image forming optical system with an optical 5' axis and having a concave, arcuate reflector sub-' tending a relatively large angle at said source and a convex, arcuate reflector subtendlng a relatively small angle at said source, said system 10 finite space and said-reflectors arranged along said axis and forming an image of said source at another point along said axis by double reflection of all light passing along said axis as far as said 1 image, first-from one reflector and then from the other reflector to said image, said source beingflnite, and said reflectors having their-reflecting surfaces as a combination corrected for both as expressed by' ing a relatively large angle at saidsource and a convex, arcuate reflector subtending a relatively small angle at said source, said system; having said source in said axis at one focus in finite space and said reflectors arranged along said axisand forming an image'oi said sourceat another point along said axis by double reflection of all light passing along said axis as far as said image,

and small in comparison to the focal length of" the system, and said reflectors having their re fleeting surfaces as a combination corrected for both spherical aberration, and coma as expressed by the sine condition, in the image, said system having an opaquewall disposed across said axis and of an area to limit light passing along said axis from said source towards said image, to that pencil of light rays which is subtended by said concave reflector.

8. An improved, image forming optical device of the type useful for headlights, projection apparatus, and microscopes, comprising a source of light, a. double reflecting, lens free, image forming 5o optical system' with a straight optical axis and having a concave, arcuate reflector subtending a relatively large angle at said source and a convex, arcuate reflector subtending a relatively small angle at said source, said. system having said source in said axis at one. focus in finite space and said reflectors arranged along said axis and forming an image of said source at another point along said axis by double reflection of all light limit light passing along said axis from said source as far as said image, to that pencil of light rays which is subtended by said concave reflector, and a spherical type concave'reflector concentric to said source, and disposed across said axis at the side of said source oppositei'rom said concave reflector for reflecting back through said source substantially all direct light from said source which is incident thereon, whereby said light which is reflected back through the source will travel forwardly along said axis in the same manneras the direct light travelling in that direction from said source.

7. An improved, image forming optical device of the type useful for headlights, projection apparatus, and microscopes, comprising a source of light, adouble reflecting, lens free, image forming optical system with a straight optical axis and having a concave, arcuate reflector subtending a relatively large angle at said source and a convex, arcuate reflector subtending a relatively small angle at said source, said system having said source in said axis at one focus in flnite space and said reflectors arranged along said axis and forming an image of said source at another point along said axis by double reflection of all light passing along said axis as far as said image, first from one reflector and then from the other reflector to said image, said source being finite and small in comparison to the focal length of the system, and said reflectors having their reflecting surfaces as a combination corrected for both spherical aberration, and coma as expressed by the sine condition, in the image, said system having an opaque wall disposed across said axis and of an area to limit light passing along said axis from said source to said image, to that pencil of light rays which is subtended by said concave reflector, both of said reflectors representing surfaces ofv revolution, with said optical axis as the axis of generation of said surfaces.

and with one end of said concave reflector extending approximately to a plane through said source and normal to said axis, and with said convex reflector being disposed approximately in the space between the ends of said concave reflector, measured along said axis.

straight optical axis and having a concave, arcu- -as expressed by the sine condition, in the image, and a spherical type concave reflector concentric 8. improved, image forming optical device comprising a source of light, a double reflecting, lens free, image forming opticalsystem with a ate reflector subtending a relatively large angle at said source and a convex, arcuate reflector subtending a relatively small angle at said source, said system having said source in said axis at one focus in finite space and said reflectors arranged along said axis and forming an image of 10 said source at another point along said axis by double reflection of all light passing along said axis as far as said image, first from one reflector and then from the other reflector to said image, said source being finite, and said reflectors having i their reflecting surfaces as a combination corrected for both spherical aberration, and coma to said source, and disposed across said axis at 20 4 the side of said source opposite from said concave reflector for reflecting back through said source substantially all direct light from Said source which is incident thereon, where'ry 583d light which is reflected back through thesource a will travel forwardly along said axis in the same manner as the direct light travelling n that direction from said source. i

9. An improved image forming device comp ing a finite source of light, a double reflecting, 30 image forming optical system with an optical axis and having a concave, arcuate reflector and I a convex, arcuate reflector, said system having said source in said axis at one focus in fails. space and said reflectors being axially aligned and arranged along said axis and subtendin? angles at said source sufflcient to reflect all ligh; from said source passing along said axis as far as said image, first from one reflector and then from the other to form said image at another 40 point along said axis by double reflection, and said reflectors having their reflecting surfaces a5,-

a combination corrected both for spherical ebsrration, and for coma as expressed b the sine condition in the image.

HAIZRY G. O'lT. 

